activity
20242026
collaborators

12 papers

astro-ph.GA2026

An Old, Low-mass, Metal-poor Hypervelocity Star Candidate Consistent with a Galactic Center Origin

Shunhong Deng, Yang Huang, Haozhu Fu +4

We report the discovery of DESI-HVS1, a hypervelocity star (HVS) candidate identified from DESI DR1 spectroscopy and Gaia DR3 astrometry. DESI-HVS1 is an old, low-mass, metal-poor…

astro-ph.SR2026

GSC 08227-00723: An Unusually Large PSH Excess AH Pic Candidate

Xin Li, Yongkang Sun

Nova-like variables are high-accretion-rate cataclysmic variables (CVs) that, in contrast to dwarf novae, do not undergo outbursts caused by thermal-viscous instability. However, a…

astro-ph.HE2025

IGR J17091-3624: Newly Formed Periodic Dips and Multiwavelength Activity During the 2025 Outburst

Zikun Lin, Yanan Wang, Shuyuan Wei +15

The black hole low-mass X-ray binary (LMXB) candidate IGR J17091-3624 experienced a hard-state-only outburst in 2025. In this paper, we show that IXPE detected a series of intermit…

astro-ph.GA2025

Systematic search for blue hyper-velocity stars from LAMOST survey

Yongkang Sun, Yang Huang, Jifeng Liu +6

Hypervelocity stars (HVSs) represent a unique class of objects capable of escaping the gravitational pull of the Milky Way due to extreme acceleration events, such as close encount…

astro-ph.IM2025

The Mini-SiTian Array: Imaging Processing Pipeline

Kai Xiao, Zhirui Li, Yang Huang +19

As a pathfinder of the SiTian project, the Mini-SiTian (MST) array, employed three commercial CMOS cameras, represents a next-generation, cost-effective optical time-domain survey…

astro-ph.HE2025

Searching for kilonova with the SiTian prototype telescope

Zhirui Li, Hongrui Gu, Yongkang Sun +3

We simulate the optical searching of gravitational-wave electromagnetic counterpart of the binary neutron star (BNS) merger event (i.e., a kilonova) using the ground based {\it SiT…